← Ishga qaytish
Ushbu ish iqtibos qilgan ishlar
32 ta ish
Ish: Asymptotic Normalization Coefficients for Proton Coupling in 12C
Determination of nuclear vertex constants (asymptotic normalization coefficients) for the virtual decays 3He → d + p and 17F → 16O + p and their use for extrapolating astrophysical S-factors of the radiative proton capture by the deuteron and the 16O nucleus at very low energies
S. V. Artemov, S. B. Igamov, K. I. Tursunmakhatov +1
MaqolaNuclear physics research studiesBulletin of the Russian Academy of Sciences Physics20098 iqtibosABISimple optical model treatment of the elastic 3He scattering
H.J. Trost, P. Lezoch, U. Strohbusch
Maqola19876 iqtibosABIThe (d, n) reaction on 1p shell nuclei at Ed = 11.8 MeV
G. S. Mutchler, D. Rendić, Donald E. Velkley +2
Maqola19714 iqtibosABIA global nucleon optical model potential
R. L. Varner, William J. Thompson, T.L. McAbee +2
Maqola19914 iqtibosABIAsymptotic normalization coefficient for $${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$ from the $${}^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$ reaction and the $${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$ astrophysical S factor
S. V. Artemov, R. Yarmukhamedov, N. Burtebayev +22
ABIComparaison des réactions (d, 3He) ET (d, t) sur quelques noyaux N = Z
M. J. Gaillard, R. Bouché, L. Feuvrais +5
Maqola19683 iqtibosABITransfer reaction code with nonlocal interactions
L. J. Titus, A. Ross, F. M. Nunes
Maqola20162 iqtibosABI<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math> proton-transfer reactions on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>9</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mo> </mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>11</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mo> </mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>13</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mo> </mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">N</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>14</mml:mn><mml:mo>,</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>, and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">F</mml:mi><mml:mprescripts/><mml:none/><mml:mn>19</mml:mn></mml:mmultiscripts></mml:math> and spectroscopic factors at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi>d</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn>16</mml:mn><mml:mspace width="0.16em"/><mml:mi>MeV</mml:mi></mml:mrow></mml:math>
M. Febbraro, F.D. Becchetti, R. O. Torres-Isea +4
Maqola20172 iqtibosABISignatures of inhomogeneity in the early universe
Lawrence Kawano, William A. Fowler, Ralph W. Kavanagh +1
Maqola19912 iqtibosABI